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Colloquium by Shude Mao (NAOC/Tsinghua)

Dynamical modelling of the Milky Way  and Nearby Galaxies


An understanding of the dynamics of galaxies provides strong clues how other galaxies form and evolve. I will report some of our dynamical works, including the study of substructure and local dark matter density in the Milky Way, and of nearby galaxies, including the mass-to-light ratio gradients and the calibrations of the Jeans Anisotropic Method obtained from IFU data.

Time: Dec. 2,  2015, 2:30 pm

Venue: A601, NAOC